Results 51 to 60 of about 1,957 (169)

Size Growth on Short Timescales of Star-forming Galaxies: Insights from Size Variation with Rest-frame Wavelength with JADES

open access: yesThe Astrophysical Journal
We investigate size variation with rest-frame wavelength for star-forming galaxies based on the second James Webb Space Telescope Advanced Deep Extragalactic Survey data release.
Cheng Jia   +13 more
doaj   +1 more source

Colour distributions in E-S0 galaxies. [PDF]

open access: yesAstronomy and Astrophysics Supplement Series, 2000
Colours distributions have been studied in 12 S0 galaxies, most of these nearly edge-on, from high resolution frames obtained at the CFHT and the Pic du Midi 2 m telescope, supplemented for some purposes by low resolution frames from the Observatoire de Haute Provence 120 cm telescope.
R. Michard, P. Poulain
openaire   +1 more source

Structural and Morphological Properties of Ultraluminous Infrared Galaxies at 1 < z < 3

open access: yesOpen Astronomy, 2015
Using the Hubble Space Telescope (HST)/Wide Field Camera 3 (WFC3) near-infrared high-resolution imaging from the 3D-HST survey, we analyze the morphology and structure of 502 ultraluminous infrared galaxies (ULIRGs; LIR > 1012L⊙) at 1 < z < 3. Their rest-
Fang Guanwen   +3 more
doaj   +1 more source

Characterizing the Average Interstellar Medium Conditions of Galaxies at z ∼ 5.6–9 with Ultraviolet and Optical Nebular Lines

open access: yesThe Astrophysical Journal
Ultraviolet (UV; rest-frame ∼1200–2000 Å) spectra provide a wealth of diagnostics to characterize fundamental galaxy properties, such as their chemical enrichment, the nature of their stellar populations, and their amount of Lyman-continuum (LyC ...
Weida Hu   +32 more
doaj   +1 more source

SQuIGG E: Buried Star Formation Cannot Explain the Rapidly Fading CO(2–1) Luminosity in Massive, z ∼ 0.7 Post-starburst Galaxies

open access: yesThe Astronomical Journal
Observational and theoretical studies have long held that rapid gas consumption in starbursts is responsible for the formation of the most massive quiescent galaxies at high redshift.
David J. Setton   +14 more
doaj   +1 more source

SAURON: Observations of E/S0/Sa galaxies

open access: yes, 2002
We present results from a new and unique integral-field spectrograph, SAURON. It has a large field of view and high throughput and is primarily built for the study of stellar & gaseous kinematics and stellar populations in galaxies. Its aim is to carry out a systematic survey of the velocity fields, velocity dispersions, and line-strength ...
Kuntschner, H   +11 more
openaire   +3 more sources

Colour distributions in E-S0 galaxies [PDF]

open access: yesAstronomy and Astrophysics Supplement Series, 1999
The colours distributions (with R in Cousins's system) have been measured in 44 E classified galaxies in the Local Supercluster, from pairs of frames collected by Nieto and co-workers in 1989-91. These are nearly all from the CFHT, and of sub-arsec resolution.
openaire   +1 more source

The Hα Concentration of Local Star-forming Galaxies: Implications for Galaxy Structure Formation

open access: yesThe Astrophysical Journal
In this work, we present a study on the H α emission line flux concentration of 3098 low-redshift star-forming galaxies (SFGs) using the MaNGA data available in the Data Release 17 from the Sloan Digital Sky Survey (SDSS).
Zhizheng Pan, Xianzhong Zheng, Xu Kong
doaj   +1 more source

Morphological Demographics of Galaxies at z ∼ 10–16: Log-normal Size Distribution and Exponential Profiles Consistent with the Disk Formation Scenario

open access: yesThe Astrophysical Journal
We homogeneously investigate the morphological properties of 169 galaxies at z  ∼ 10–16 with deep JWST NIRCam images employing our established techniques of GALFIT modeling and uncertainty evaluation (systematics+statistics).
Yoshiaki Ono   +7 more
doaj   +1 more source

Blue E/S0 galaxies: merger remnants or disk rebuilding galaxies?

open access: yes, 2009
This paper has been withdrawn A new version is in preparation and will be soon available.
Aguerri, J. A. L.   +2 more
openaire   +2 more sources

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